A relativistic formalism for computation of irrotational binary stars in quasi equilibrium states

Details A relativistic formalism for computation of irrotational binary stars in quasi equilibrium states A relativistic formalism for computation of irrotational binary stars in quasi equilibrium states

1998-03-26

arxiv.org/abs/gr-qc/9803085v3

Phys.Rev. D58 (1998) 024012

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

5 pages, corrected eqs.(2.10), (2.11) and (3.1)

Scientific paper

10.1103/PhysRevD.58.024012

We present relativistic hydrostatic equations for obtaining irrotational binary neutron stars in quasi equilibrium states in 3+1 formalism. Equations derived here are different from those previously given by Bonazzola, Gourgoulhon, and Marck, and have a simpler and more tractable form for computation in numerical relativity. We also present hydrostatic equations for computation of equilibrium irrotational binary stars in first post-Newtonian order.

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